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A case for Case A: Detailed look at binary black hole formation through stable mass transfer

Context. In isolated binary evolution, binary black hole (BBH) mergers are generally formed through stable mass transfer (SMT) or common envelope evolution. In recent years, the SMT channel has received significant attention due to detailed binary models showing increased mass transfer stability com...

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Principais autores: Briel Max M., Fragos Tassos, Gallegos-Garcia Monica, Ray Anarya, Zevin Michael, Chattaraj Abhishek, Andrews Jeff J., Kalogera Vicky, Gossage Seth, Srivastava Philipp M., Teng Elizabeth
Formato: Artigo
Idioma:Inglês
Publicado em: EDP Sciences 2026-06-01
coleção:Astronomy & Astrophysics
Assuntos:
gravitational waves
binaries: close
stars: black holes
stars: massive
Acesso em linha:https://www.aanda.org/articles/aa/full_html/2026/06/aa59298-26/aa59298-26.html
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